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X-RAY OBSERVATIONS.GIACCONI R.1976; IN: PHYS. NON-THERM. RADIO SOURCES. NATO ADV. STUDY INST. PROC.; URBINO; 1975; DORDRECHT; D. REIDEL; DA. 1976; PP. 229-269; BIBL. 2 P.Conference Paper

ETUDE ET REALISATION D'UN ENSEMBLE DE PROGRAMMATION ET DE TRAITEMENT DE DONNEES COMMUN AUX METHODES SPECTROMETRIQUES ET DIFFRACTOMETRIQUES DES RAYONS XD'HAENNENS M; TOURNIER M.1978; ; FRA; DA. 1978; DGRST-7670818; (45) P.: ILL.; 30 CM; ACTION CONCERT.: INSTRUM. MES.Report

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SPECTRAL CHARACTERISTICS OF TRANSIENT X-RAY SOURCES.MARASCHI L; HUCKLE HE; IVES JC et al.1976; NATURE; G.B.; DA. 1976; VOL. 263; NO 5572; PP. 34-36; BIBL. 25 REF.Article

INTENSITY AND SPECTRAL VARIABILITY OF STRONG GALACTIC X-RAY SOURCES OBSERVED BY ANSPARSIGNAULT DR; GRINDLAY JE.1978; ASTROPHYS. J.; USA; DA. 1978; VOL. 225; NO 3 PART. 1; PP. 970-987; BIBL. 41 REF.Article

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Measurement of cross sections for ²²Na, ^20-22Ne and ^36-42Ar in the spallation of Mg, Al, Si, Ca and Fe: production ratios of some cosmogenic nuclides in meteorites = Mesure de sections efficaces pour ²²Na, ²⁰-²²Ne et ^36-42Ar dans la spallation de Mg, Al, Si, CA et Fe. Rapports de production de certains nuclides cosmogéniques dans des météoritesBAROS, F; REGNIER, S.Journal de physique (Paris). 1984, Vol 45, Num 5, pp 855-861, issn 0302-0738Article

Measurement of cosmogenic radionuclides in meteorites with a sensitive gamma-ray spectrometerBONINO, G; CINI CASTAGNOLI, G; BHANDARI, N et al.Nuovo cimento della società italiana di fisica. C. 1992, Vol 15, Num 1, pp 99-104, issn 0390-5551Article

Components of the 11- and 22-year variation of cosmic raysPOPIELAWSKA, B.Planetary and space science. 1992, Vol 40, Num 6, pp 811-827, issn 0032-0633Article

THE ISOTOPIC AND ELEMENTAL ABUNDANCES OF NEON NUCLEI ACCELERATED IN SOLAR FLARESDIETRICH WF; SIMPSON JA.1979; ASTROPHYS. J.; USA; DA. 1979; VOL. 231; NO 2 PART. 2; PP. L91-L95; BIBL. 31 REF.Article

On the cosmogenic radionuclides in meteoritesBONINO, G; CINI CASTAGNOLI, G; TARICCO, C et al.Nuovo cimento della società italiana di fisica. C. 1995, Vol 18, Num 4, pp 411-418, issn 0390-5551Article

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